The magnitude of the expected superfluid transition temperature and the form of the gap are obtained for regimes of neutron density expected in neutron-star cores. For neutron densities exceeding 1.5×{}10¹⁴ g cm^-3 the gap is anisotropic but nodeless, leading to thermodynamic properties of a conventional BCS-type superfluid.
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Hoffberg et al. (1970) studied this question.
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